Zobrazeno 1 - 10
of 4 361
pro vyhledávání: '"Klement, P."'
Autor:
Rivinius, Thomas, Klement, Robert
Classical Be stars, the "e" standing for the presence of spectroscopic line emission, are main sequence stars of spectral type B that are able to form a gaseous disk in Keplerian motion from star-ejected matter. The main driver of this capability is
Externí odkaz:
http://arxiv.org/abs/2411.06882
Autor:
Pálka, Petr, Landini, Federico, Klement, Dominik, Diez, Mireia, Silnova, Anna, Delcroix, Marc, Burget, Lukáš
In spite of the popularity of end-to-end diarization systems nowadays, modular systems comprised of voice activity detection (VAD), speaker embedding extraction plus clustering, and overlapped speech detection (OSD) plus handling still attain competi
Externí odkaz:
http://arxiv.org/abs/2411.02165
Autor:
Patel, D. K., Fijalkowski, K. M., Kruskopf, M., Liu, N., Götz, M., Pesel, E., Jaime, M., Klement, M., Schreyeck, S., Brunner, K., Gould, C., Molenkamp, L. W., Scherer, H.
The quantum anomalous Hall effect holds promise as a disruptive innovation in condensed matter physics and metrology, as it gives access to Hall resistance quantization in terms of the von-Klitzing constant RK = h/e2 at zero external magnetic field.
Externí odkaz:
http://arxiv.org/abs/2410.13365
Autor:
Polok, Alexander, Klement, Dominik, Wiesner, Matthew, Khudanpur, Sanjeev, Černocký, Jan, Burget, Lukáš
We propose a novel approach to enable the use of large, single speaker ASR models, such as Whisper, for target speaker ASR. The key insight of this method is that it is much easier to model relative differences among speakers by learning to condition
Externí odkaz:
http://arxiv.org/abs/2409.09543
Autor:
Torres, Guillermo, Schaefer, Gail H., Stefanik, Robert P., Latham, David W., Boden, Andrew F., Anugu, Narsireddy, Jones, Jeremy W., Klement, Robert, Kraus, Stefan, Lanthermann, Cyprien, Monnier, John D.
We report long baseline interferometric observations with the CHARA Array that resolve six previously known double-lined spectroscopic binary systems in the Hyades cluster, with orbital periods ranging from 3 to 358 days: HD 27483, HD 283882, HD 2687
Externí odkaz:
http://arxiv.org/abs/2406.01674
In this paper, we investigate the security implications of virtualized and software-based Open Radio Access Network (RAN) systems, specifically focusing on the architecture proposed by the O-RAN ALLIANCE and O-Cloud deployments based on the O-RAN Sof
Externí odkaz:
http://arxiv.org/abs/2405.01888
Autor:
Fijalkowski, Kajetan M., Liu, Nan, Klement, Martin, Schreyeck, Steffen, Brunner, Karl, Gould, Charles, Molenkamp, Laurens W.
Publikováno v:
Nature Electronics (2024)
The quantum anomalous Hall effect in magnetic topological insulators has been recognized as a promising platform for applications in quantum metrology. The primary reason for this is the electronic conductance quantization at zero external magnetic f
Externí odkaz:
http://arxiv.org/abs/2402.04126
Autor:
Klement, Robert, Rivinius, Thomas, Gies, Douglas R., Baade, Dietrich, Merand, Antoine, Monnier, John D., Schaefer, Gail H., Lanthermann, Cyprien, Anugu, Narsireddy, Kraus, Stefan, Gardner, Tyler
Rapid rotation and nonradial pulsations enable Be stars to build decretion disks, where the characteristic line emission forms. A major but unconstrained fraction of Be stars owe their rapid rotation to mass and angular-momentum transfer in a binary.
Externí odkaz:
http://arxiv.org/abs/2312.08252
Autor:
Klement, Dominik, Diez, Mireia, Landini, Federico, Burget, Lukáš, Silnova, Anna, Delcroix, Marc, Tawara, Naohiro
Bayesian HMM clustering of x-vector sequences (VBx) has become a widely adopted diarization baseline model in publications and challenges. It uses an HMM to model speaker turns, a generatively trained probabilistic linear discriminant analysis (PLDA)
Externí odkaz:
http://arxiv.org/abs/2310.02732
Autor:
Rubio, A. C., Carciofi, A. C., Ticiani, P., Mota, B. C., Vieira, R. G., Faes, D. M., Genaro, M., de Amorim, T. H., Klement, R., Araya, I., Arcos, C., Curé, M., de Souza, A. Domiciano, Georgy, C., Jones, C. E., Suffak, M. W., Silva, A. C. F.
Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars. Our goal is to infer stellar and disc parameters, as well as distance an
Externí odkaz:
http://arxiv.org/abs/2309.06168